The reduction on the linear stability of elliptic Euler-Moulton solutions of the n-body problem to those of 3-body problems

TL;DR

This paper reduces the linear stability analysis of elliptic Euler-Moulton collinear solutions in the n-body problem to the stability of corresponding 3-body solutions, simplifying the complex n-body problem analysis.

Contribution

It proves that the linearized Hamiltonian system for n-body elliptic Euler-Moulton solutions decomposes into independent systems linked to 3-body problems, enabling easier stability analysis.

Findings

Linearized system splits into (n-1) independent Hamiltonian systems.

The stability of n-body solutions reduces to 3-body problem stability.

Detailed stability analysis provided for a 4-body case with two small masses.

Abstract

In this paper, we consider the elliptic collinear solutions of the classical $n$-body problem, where the $n$ bodies always stay on a straight line, and each of them moves on its own elliptic orbit with the same eccentricity. Such a motion is called an elliptic Euler-Moulton collinear solution. Here we prove that the corresponding linearized Hamiltonian system at such an elliptic Euler-Moulton collinear solution of $n$-bodies splits into $(n-1)$ independent linear Hamiltonian systems, the first one is the linearized Hamiltonian system of the Kepler $2$-body problem at Kepler elliptic orbit, and each of the other $(n-2)$ systems is the essential part of the linearized Hamiltonian system at an elliptic Euler collinear solution of a $3$-body problem whose mass parameter is modified. Then the linear stability of such a solution in the $n$-body problem is reduced to those of the corresponding elliptic Euler collinear solutions of the $3$-body problems, which for example then can be further understood using numerical results of Martin\'ez, Sam\`a and Sim\'o in \cite{MSS1} and \cite{MSS2} on $3$-body Euler solutions in 2004-2006. As an example, we carry out the detailed derivation of the linear stability for an elliptic Euler-Moulton solution of the $4$-body problem with two small masses in the middle.